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Gabriela Oliveira da Rosa

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
ORCID 0009-0009-6670-0943

identity via Semantic Scholar / OpenAlex

most citedPhotometric White Dwarf Rotation

11 citations · 21 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024

Thirty Two New Bright ZZ Ceti Stars from TESS: Adding Cycles 4 and 5

Alejandra D. Romero, S. O. Kepler, Gabriela Oliveira da Rosa +1

Analyzing all 120 s and 20 s light curves obtained by the TESS satellite up to Sector 69 - the end of the fifth year of observations - for all known white dwarfs and white dwarf ca…

astro-ph.SR2024★ 11 cited

Photometric White Dwarf Rotation

Gabriela Oliveira da Rosa, S. O. Kepler, L. T. T. Soethe +2

We present a census of photometrically detected rotation periods for white dwarf (WD) stars. We analyzed the light curves of 9285 WD stars observed by the Transiting Exoplanet Surv…

astro-ph.SR2022★ 10 cited

Kepler and TESS Observations of PG 1159-035

Gabriela Oliveira da Rosa, S. O. Kepler, Alejandro H. Córsico +11

PG 1159-035 is the prototype of the DOV hot pre-white dwarf pulsators. It was observed during the Kepler satellite K2 mission for 69 days in 59 s cadence mode and by the TESS satel…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.